Orbit Fit and Astrometric record for 543376

The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory. Take special note that while the original Bernstein software works with barycentric coordinates, we convert these results into a heliocentric coordinate system.

# Object: 543376    
# Created Fri Apr 26 01:08:46 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     81 observations of     81
# Arc:   9.18y
# First observation: 2014/01/21
#  Last observation: 2023/03/27
# Chi-squared of fit:    59.94 DOF:    156 RMS:  0.15
# Min/Max residuals:    -0.53    0.56
# Exact a, adot, b, bdot, g, gdot:
  2.028064E-05  3.153034E-02 -1.014758E-06 -1.187508E-03  2.532404E-02 -4.413734E-03
# Covariance matrix:
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
#      lat0       lon0       xBary       yBary       zBary        JD0
  -25.892597  144.775814    0.393510   -0.392622   -0.809109  2456678.963918
# Heliocentric elements and errors
Epoch:              2456678.5000  =  2014/01/21
Mean Anomaly:          356.07026 +/-     0.000
Argument of Peri:      287.11061 +/-     0.000
Long of Asc Node:      239.55761 +/-     0.000
Inclination:            25.43042 +/-     0.000
Eccentricity:         0.63130080 +/-    0.0000
Semi-Major Axis:    106.23358780 +/-    0.0000
Time of Perihelion: 2461044.1843 +/-       0.0
Perihelion:          39.16823909 +/-    0.0000
Aphelion:           173.29893652 +/-    0.0000
Period (y)             1094.9669 +/-      0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -29.52896922 +/-    0.0000
Ecliptic Y           21.33124428 +/-    0.0000
Ecliptic Z          -17.24397309 +/-    0.0000
Ecliptic XDOT        -0.00157564 +/-    0.0000
Ecliptic YDOT        -0.00306718 +/-    0.0000
Ecliptic ZDOT         0.00009302 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.30317524 +/-    0.0000
Geocenter to KBO     39.48831235 +/-    0.0000
# Hcoef:  5.95

The following table shows the complete astrometric record for 543376. The first three columns show the date of observation. The next six columns are RA and DEC. The next column (when provided) is the observed magnitude and filter. The next column is the object name (543376) followed by the observatory code and reference code for the source of the astrometry.

2014 01  21.46314  09 14 04.382  -11 12 04.08  21.9G 543376    F51  C~346O      
2014 01  21.47567  09 14 04.328  -11 12 03.77  21.9G 543376    F51  C~346O      
2014 03  09.33393  09 10 31.096  -10 54 28.33  21.2G 543376    F51  C~346O      
2014 04  28.25090  09 08 55.057  -10 22 13.91  21.7G 543376    F51  C~346O      
2014 04  28.25159  09 08 55.060  -10 22 14.04  21.9G 543376    F51  C~346O      
2014 04  28.26424  09 08 55.063  -10 22 13.64  21.8G 543376    F51  C~346O      
2014 04  28.26493  09 08 55.064  -10 22 13.46  22.2G 543376    F51  C~346O      
2014 04  28.27752  09 08 55.050  -10 22 13.25  22.1G 543376    F51  C~346O      
2014 04  28.27822  09 08 55.065  -10 22 13.02  21.9G 543376    F51  C~346O      
2014 04  28.29084  09 08 55.061  -10 22 12.67  21.9G 543376    F51  C~346O      
2014 04  28.29153  09 08 55.057  -10 22 12.27  21.8G 543376    F51  C~346O      
2014 12  01.65595  09 23 34.825  -11 38 02.55  23.1G 543376    F51  C~346O      
2014 12  27.67294  09 22 38.829  -11 49 24.06  20.3G 543376    F51  C~346O      
2015 01  24.44680  09 20 46.980  -11 51 28.23  22.9G 543376    F51  C~346O      
2015 01  24.45809  09 20 46.925  -11 51 28.04  22.2G 543376    F51  C~346O      
2015 01  24.46940  09 20 46.873  -11 51 28.04  21.9G 543376    F51  C~346O      
2015 01  24.48072  09 20 46.812  -11 51 27.86  21.9G 543376    F51  C~346O      
2015 01  26.41662  09 20 37.810  -11 51 12.21  21.7G 543376    F51  C~346O      
2015 01  26.42807  09 20 37.754  -11 51 12.08  21.8G 543376    F51  C~346O      
2015 01  26.43957  09 20 37.701  -11 51 12.03  21.7G 543376    F51  C~346O      
2015 04  13.24877  09 15 50.426  -11 11 33.91  22.1G 543376    F51  C~346O      
2015 04  13.25937  09 15 50.409  -11 11 33.55  22.0G 543376    F51  C~346O      
2015 04  13.27001  09 15 50.393  -11 11 32.87  21.8G 543376    F51  C~346O      
2015 04  13.28062  09 15 50.382  -11 11 32.62  22.1G 543376    F51  C~346O      
2015 04  21.28915  09 15 43.073  -11 06 13.53  22.2G 543376    F51  C~346O      
2016 01  15.49177  09 28 28.299  -12 31 20.05  22.0G 543376    F51  C~346O      
2016 01  15.50345  09 28 28.228  -12 31 20.15  22.0G 543376    F51  C~346O      
2016 01  15.51513  09 28 28.185  -12 31 20.08  21.7G 543376    F51  C~346O      
2016 01  15.52683  09 28 28.146  -12 31 19.99  22.0G 543376    F51  C~346O      
2016 01  17.47464  09 28 19.810  -12 31 21.04  21.7G 543376    F51  C~346O      
2016 01  17.48596  09 28 19.765  -12 31 21.11  21.8G 543376    F51  C~346O      
2016 01  17.49726  09 28 19.712  -12 31 21.16  21.8G 543376    F51  C~346O      
2016 01  17.50865  09 28 19.669  -12 31 20.97  21.9G 543376    F51  C~346O      
2016 02  12.44615  09 26 18.597  -12 26 33.30  22.2G 543376    F51  C~346O      
2016 02  12.45843  09 26 18.541  -12 26 33.37  21.8G 543376    F51  C~346O      
2016 02  12.47072  09 26 18.473  -12 26 32.94  22.0G 543376    F51  C~346O      
2016 02  12.48300  09 26 18.421  -12 26 32.56  21.9G 543376    F51  C~346O      
2016 02  25.45065  09 25 17.437  -12 21 00.36  22.5G 543376    F51  C~346O      
2016 03  03.34413  09 24 46.905  -12 17 22.53  21.8G 543376    F51  C~346P      
2016 03  03.34477  09 24 46.901  -12 17 22.61  21.7G 543376    F51  C~346P      
2016 03  03.35579  09 24 46.857  -12 17 22.14  21.9G 543376    F51  C~346P      
2016 03  03.35643  09 24 46.842  -12 17 22.16  21.9G 543376    F51  C~346P      
2016 03  03.36744  09 24 46.798  -12 17 21.81  21.8G 543376    F51  C~346P      
2016 03  03.36808  09 24 46.801  -12 17 21.78  22.0G 543376    F51  C~346P      
2016 03  03.37909  09 24 46.741  -12 17 21.39  21.9G 543376    F51  C~346P      
2016 03  03.37974  09 24 46.746  -12 17 21.31  22.0G 543376    F51  C~346P      
2016 03  14.33189  09 24 02.637  -12 10 49.30  20.4G 543376    F51  C~346P      
2016 04  01.31676  09 23 06.822  -11 58 48.25  22.1G 543376    F51  C~346P      
2016 04  01.32922  09 23 06.797  -11 58 47.75  22.0G 543376    F51  C~346P      
2016 04  01.34132  09 23 06.768  -11 58 47.26  21.7G 543376    F51  C~346P      
2016 04  01.35341  09 23 06.737  -11 58 46.73  21.8G 543376    F51  C~346P      
2016 04  12.27440  09 22 45.455  -11 51 13.21  21.9G 543376    F51  C~346P      
2017 03  04.38845  09 31 48.581  -12 56 24.89  22.0G 543376    F51  C~346P      
2017 03  04.40017  09 31 48.530  -12 56 24.43  21.8G 543376    F51  C~346P      
2017 03  04.41189  09 31 48.469  -12 56 24.01  22.5G 543376    F51  C~346P      
2017 03  04.42365  09 31 48.427  -12 56 23.20  21.4G 543376    F51  C~346P      
2017 03  13.37357  09 31 11.477  -12 51 03.38  22.4G 543376    F51  C~346P      
2017 12  04.58848  09 44 29.838  -13 34 25.36  21.8G 543376    F51  C~346P      
2017 12  14.58606  09 44 17.466  -13 39 58.34  22.2G 543376    F51  C~346P      
2017 12  26.52455  09 43 50.702  -13 44 58.38  22.2G 543376    F51  C~346P      
2017 12  26.53659  09 43 50.666  -13 44 58.68  22.0G 543376    F51  C~346P      
2017 12  26.54863  09 43 50.634  -13 44 58.87  21.7G 543376    F51  C~346P      
2017 12  26.56067  09 43 50.601  -13 44 59.26  22.0G 543376    F51  C~346P      
2020 01  19.55072  09 57 00.581  -15 04 25.27  21.7w 543376    F51  C~3cm8      
2020 01  19.56251  09 57 00.524  -15 04 25.20  21.7w 543376    F51  C~3cm8      
2020 01  19.57428  09 57 00.476  -15 04 25.27  21.7w 543376    F51  C~3cm8      
2020 01  19.58606  09 57 00.425  -15 04 25.40  21.8w 543376    F51  C~3cm8      
2021 04  07.297007 09 58 48.694  -15 06 42.19  21.9w 543376    F51  C~4mnn      
2021 04  07.308794 09 58 48.651  -15 06 41.55  21.8w 543376    F51  C~4mnn      
2021 04  07.320598 09 58 48.629  -15 06 40.88  21.8w 543376    F51  C~4mnn      
2021 04  07.332411 09 58 48.593  -15 06 40.52  21.8w 543376    F51  C~4mnn      
2022 03  02.241330 10 08 37.532  -16 06 51.33  21.7G 543376    G37  C~5V48      
2022 03  02.298230 10 08 37.244  -16 06 49.19        543376    G37  C~5V48      
2022 03  02.350880 10 08 37.000  -16 06 47.33        543376    G37  C~5V48      
2022 12  01.610034 10 20 48.333  -16 30 38.28  21.9w 543376    F51  C~69R2      
2022 12  01.620355 10 20 48.354  -16 30 38.50  21.8w 543376    F51  C~69R2      
2022 12  01.630707 10 20 48.365  -16 30 38.93  21.7w 543376    F51  C~69R2      
2022 12  01.641031 10 20 48.380  -16 30 39.43  21.8w 543376    F51  C~69R2      
2023 03  27.334310 10 14 22.307  -16 27 04.89  21.6w 543376    F52  C~6hCW      
2023 03  27.345758 10 14 22.263  -16 27 04.33  21.5w 543376    F52  C~6hCW      
2023 03  27.368659 10 14 22.163  -16 27 03.53  21.8w 543376    F52  C~6hCW      

The following table shows the residuals to the orbit fit. The first coumn is the point number. The second column is the time, in years, measured from the first observation. The third and fifth columns are the regularized positions used in the orbit fit. The fourth and sixth columns are the residuals, in arc seconds, for RA and Dec respectively.

     1   0.0000      0.00    -0.10       0.00     0.09
     2   0.0000      0.00    -0.03       0.00     0.33
     3   0.1283      0.00    -0.37       0.00    -0.11
     4   0.2650      0.00     0.01       0.00     0.08
     5   0.2650      0.00     0.05       0.00    -0.07
     6   0.2650      0.00     0.05       0.00    -0.13
     7   0.2650      0.00     0.07       0.00     0.03
     8   0.2651      0.00    -0.19       0.00    -0.22
     9   0.2651      0.00     0.03       0.00    -0.01
    10   0.2651      0.00    -0.07       0.00    -0.12
    11   0.2651      0.00    -0.13       0.00     0.25
    12   0.8602      0.00     0.48       0.00     0.12
    13   0.9314      0.00     0.56       0.00     0.48
    14   1.0075      0.00     0.13       0.00    -0.12
    15   1.0075      0.00     0.10       0.00    -0.01
    16   1.0075      0.00     0.12       0.00    -0.10
    17   1.0076      0.00     0.01       0.00     0.00
    18   1.0129      0.00    -0.10       0.00    -0.10
    19   1.0129      0.00    -0.12       0.00    -0.07
    20   1.0129      0.00    -0.09       0.00    -0.12
    21   1.2232      0.00    -0.04       0.00    -0.02
    22   1.2233      0.00    -0.08       0.00    -0.08
    23   1.2233      0.00    -0.09       0.00     0.17
    24   1.2233      0.00    -0.04       0.00    -0.01
    25   1.2452      0.00     0.34       0.00     0.13
    26   1.9823      0.00     0.08       0.00    -0.06
    27   1.9823      0.00    -0.23       0.00    -0.14
    28   1.9823      0.00    -0.11       0.00    -0.06
    29   1.9824      0.00     0.06       0.00     0.05
    30   1.9877      0.00    -0.08       0.00     0.04
    31   1.9877      0.00    -0.01       0.00    -0.03
    32   1.9878      0.00    -0.05       0.00    -0.09
    33   1.9878      0.00     0.05       0.00     0.10
    34   2.0588      0.00    -0.10       0.00     0.13
    35   2.0589      0.00    -0.04       0.00    -0.21
    36   2.0589      0.00    -0.16       0.00    -0.04
    37   2.0589      0.00    -0.04       0.00     0.08
    38   2.0944      0.00    -0.17       0.00    -0.17
    39   2.1133      0.00     0.01       0.00     0.00
    40   2.1133      0.00    -0.00       0.00    -0.10
    41   2.1133      0.00     0.06       0.00     0.01
    42   2.1133      0.00    -0.12       0.00    -0.04
    43   2.1134      0.00    -0.06       0.00    -0.05
    44   2.1134      0.00     0.03       0.00    -0.04
    45   2.1134      0.00    -0.15       0.00    -0.02
    46   2.1134      0.00    -0.03       0.00     0.04
    47   2.1434      0.00    -0.22       0.00    -0.03
    48   2.1926      0.00    -0.08       0.00     0.06
    49   2.1927      0.00     0.02       0.00     0.04
    50   2.1927      0.00     0.04       0.00     0.03
    51   2.1927      0.00     0.03       0.00     0.06
    52   2.2226      0.00     0.46       0.00     0.00
    53   3.1155      0.00     0.04       0.00    -0.09
    54   3.1155      0.00     0.05       0.00    -0.03
    55   3.1155      0.00    -0.08       0.00    -0.00
    56   3.1156      0.00     0.07       0.00     0.41
    57   3.1401      0.00     0.28       0.00     0.41
    58   3.8689      0.00    -0.12       0.00    -0.43
    59   3.8963      0.00    -0.19       0.00    -0.16
    60   3.9290      0.00    -0.04       0.00     0.07
    61   3.9290      0.00    -0.07       0.00     0.02
    62   3.9291      0.00    -0.03       0.00     0.07
    63   3.9291      0.00    -0.01       0.00    -0.07
    64   5.9934      0.00     0.02       0.00    -0.06
    65   5.9934      0.00    -0.09       0.00     0.03
    66   5.9935      0.00    -0.07       0.00    -0.02
    67   5.9935      0.00    -0.10       0.00    -0.13
    68   7.2083      0.00     0.06       0.00    -0.02
    69   7.2083      0.00    -0.09       0.00     0.10
    70   7.2084      0.00     0.08       0.00     0.24
    71   7.2084      0.00     0.03       0.00     0.08
    72   8.1089      0.00     0.18       0.00    -0.53
    73   8.1091      0.00    -0.04       0.00    -0.13
    74   8.1092      0.00     0.10       0.00     0.11
    75   8.8601      0.00    -0.29       0.00    -0.07
    76   8.8601      0.00    -0.05       0.00     0.16
    77   8.8601      0.00     0.04       0.00     0.18
    78   8.8602      0.00     0.19       0.00     0.13
    79   9.1769      0.00     0.12       0.00    -0.01
    80   9.1770      0.00     0.12       0.00     0.06
    81   9.1770      0.00    -0.05       0.00    -0.10

The following table comes from a 10My integration of the orbit of the object. Three columns are shown. The first column is the result of integrating the nominal orbit. The other two columns are based on clones of the nominal orbit that are +/- 3 sigma from the nominal orbit. If all three types agree then the classificiation is deemed secure. The basis for these calculations is described in more detail in AJ, 129, 1117 (2005). Any use made of these calculations should refer to and credit this publication and the Deep Ecliptic Survey Team.

543376    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj       104.298   104.297   104.299
ecceobj         0.624     0.624     0.624
incobj         25.406    25.406    25.406
qmin           38.243    38.244    38.244
qmax          175.427   175.449   175.461
amean         104.428   104.427   104.428
amin          102.584   102.658   102.523
amax          107.303   107.314   107.320
emean           0.617     0.617     0.617
emin            0.604     0.604     0.604
emax            0.635     0.635     0.635
imean          27.353    27.354    27.348
imin           26.353    26.353    26.353
imax           28.192    28.193    28.191
excite_mean     0.770     0.770     0.770
fracstop        1.000     1.000     1.000
cjmean          2.891     2.891     2.891

libcent 0      -180.0    -180.0    -180.0
libamp  0      -180.0    -180.0    -180.0
libcent 1      -180.0    -180.0    -180.0
libamp  1      -180.0    -180.0    -180.0
libcent 2      -180.0    -180.0    -180.0
libamp  2      -180.0    -180.0    -180.0
libcent 3      -180.0    -180.0    -180.0
libamp  3      -180.0    -180.0    -180.0
libcent 4      -180.0    -180.0    -180.0
libamp  4      -180.0    -180.0    -180.0

kozaimean       185.5     185.2     185.4
kozaiamp        180.0     180.0     180.0